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Space Astro
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Info for exoplanet "Veluvizi"
| Scientific (actual) data |
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| Name | CD-25 11378 b |
| Planet status | Confirmed |
| Planet mass | 24.8 |
| Semi major axis | 1855 |
| Discovered | 2022 |
| Updated | 2024-10-24 |
| Publication | Published in a refereed paper |
| Detection type | Imaging, Astrometry |
| Mass measurement type | Astrometry |
| Alternate names | 2MASS J16084340-2602168 b |
| Star name | CD-25 11378 |
| Right ascension | 242.18° |
| Declination | -26.04° |
| Mag v | 10.38 |
| Mag i | 9.265 |
| Mag j | 8.55 |
| Mag h | 8.05 |
| Mag k | 7.908 |
| Star distance | 155.198 |
| Star mass | 1.135 |
| Star radius | 1.978 |
| Star sp type | G9Ve |
| Star temperature | 5045.85 |
| Star alternate names | 2MASS J16084340-2602168 |
| Wikipedia article | CD-25 11378 b |
Back
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| Fictional info (?) |
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| Suggested name | Veluvizi |
| Planet type | Huge cold gas giant |
| It is a huge cold gas giant planet with a mass one-thousandth that of CD-25 11378, but two-and-a-half times that of all the other planets in its solar system combined.
As seen from CD-25 11378, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
It may have had methane oceans in the past, but these would have vaporized as the temperature rose due to a runaway greenhouse effect.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
| Atmosphere | Ammonia | 77% |
| Ozone | 22% |
| Methane | 0.41% |
| Carbonyl sulfide | 0.035% |
| Neon | 0.016% |
| Oxygen | 0.0042% |
| Krypton | 3.0E-5% |
| Atmospheric pressure | 0.16 bar |
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| Moon | Duni Suso Jur | Medium-sized round ice comet |
| Oroh | Very small potato shaped crater-filled asteroid |
| Esur-ymuci | Very small irregular ice moon |
| Google search for Veluvizi |
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Website by Joachim Michaelis
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